Holographic hessence models
arXiv:0706.2211 · doi:10.1016/j.physletb.2007.08.083
Abstract
We discuss the evolution of holographic hessence model, which satisfies the holographic principle and can naturally realizes the equation of state crossing -1. By discussing the evolution of the models in the plane, we find that, if , and keep for all time, which are quintessence-like. However, if , which mildly favors the current observations, evolves from to , and the potential is a nonmonotonic function. In the earlier time, the potential must be rolled down, and then be climbed up. Considered the current constraint on the parameter , we reconstruct the potential of the holographic hessence model.
10 pages, 5 figures, PLB accepted
References in corpus (10)
- New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy
- Cosmological Evolution of a Quintom Model of Dark Energy
- Can dark energy evolve to the Phantom?
- Constraints on Holographic Dark Energy from Latest Supernovae, Galaxy Clustering, and Cosmic Microwave Background Anisotropy Observations
- Dynamical vacuum energy, holographic quintom, and the reconstruction of scalar-field dark energy
- Critical comments on the paper "Crossing by a single scalar field on a Dvali-Gabadadze-Porrati brane" by H Zhang and Z-H Zhu [Phys.Rev.D75,023510(2007)]
- Crossing by a single scalar on a Dvali-Gabadadze-Porrati brane
- Reconstruction of Hessence Dark Energy and the Latest Type Ia Supernovae Gold Dataset
- Interacting Energy Components and Observational Data
- Yang-Mills condensate dark energy coupled with matter and radiation
Cited by in corpus (11)
- Holographic Dark Energy in Braneworld Models with a Gauss-Bonnet Term in the Bulk. Interacting Behavior and the w =-1 Crossing
- Statefinder Diagnostic and w-w' Analysis for the Agegraphic Dark Energy Models without and with Interaction
- Quintessence reconstruction of the new agegraphic dark energy model
- Entropy-Corrected Holographic Dark Energy
- Holographic Dark Energy in Braneworld Models with Moving Branes and the w=-1 Crossing
- Holographic Ricci dark energy in Randall-Sundrum braneworld: Avoidance of big rip and steady state future
- 3-loop Yang-Mills Condensate Dark Energy Model And Its Cosmological Constraints
- Modified Holographic Dark Energy
- Statefinder diagnostic for Yang-Mills dark energy model
- Attractor Solution in Coupled Yang-Mills Field Dark Energy Models
- Dark Energy, Hyperbolic Cosecant Cardassian and Virial Collapse for Power-style Cardassian